SDO HMI 2014-10-06 18:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.33 | 203.80 | 54.20 | 195.75 | -12.18 | 165.00 | 56.13 | 251.52 | 0.8567 | 240.1 | 9.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.67 | 140.77 | 34.83 | 141.35 | -12.38 | 166.65 | 57.78 | 251.82 | 0.8717 | 646.9 | 101.4 | |
| 0.00 | 0.35 | 0.00 | 0.35 | -11.62 | 166.22 | 57.35 | 252.55 | 0.8666 | 428.0 | 392.8 | |
| 6.58 | -1.00 | 6.44 | -1.00 | -11.89 | 165.85 | 56.98 | 252.13 | 0.8641 | 754.3 | 999999 | |
| 0.79 | 2.63 | 0.76 | 2.53 | -11.50 | 165.34 | 56.47 | 252.43 | 0.8589 | 627.2 | 476.5 | |
| 0.00 | 1.05 | 0.00 | 1.00 | -11.49 | 164.95 | 56.08 | 252.32 | 0.8555 | 546.0 | 487.9 | |
| 0.00 | 1.14 | 0.00 | 1.10 | -12.45 | 165.20 | 56.33 | 251.31 | 0.8599 | 283.0 | 297.5 | |
| 0.00 | 1.32 | 0.00 | 1.29 | -14.39 | 165.33 | 56.46 | 249.19 | 0.8658 | 540.0 | 397.3 | |
| 0.00 | 0.97 | 0.00 | 0.89 | -11.82 | 163.79 | 54.92 | 251.60 | 0.8463 | -240.0 | -194.2 | |
| 0.00 | 0.97 | 0.00 | 0.88 | -11.50 | 163.38 | 54.51 | 251.83 | 0.8418 | -372.0 | -263.3 | |
| 0.00 | 1.58 | 0.00 | 1.43 | -11.90 | 162.97 | 54.10 | 251.25 | 0.8392 | 519.0 | 369.7 | |
| 0.00 | 1.58 | 0.00 | 1.42 | -11.90 | 162.65 | 53.78 | 251.14 | 0.8364 | 603.0 | 524.4 | |
| 0.00 | 0.97 | 0.00 | 0.90 | -13.97 | 163.31 | 54.44 | 248.99 | 0.8478 | -298.0 | -281.8 | |
| 1.05 | 4.56 | 0.93 | 4.04 | -11.56 | 162.09 | 53.22 | 251.35 | 0.8304 | 335.3 | 337.1 | |
| 0.00 | 1.05 | 0.00 | 0.91 | -11.25 | 161.45 | 52.58 | 251.49 | 0.8236 | -316.0 | -269.8 | |
| 1.05 | 4.65 | 0.90 | 3.99 | -11.27 | 160.95 | 52.08 | 251.31 | 0.8189 | -607.5 | -399.9 | |
| 0.00 | 2.02 | 0.00 | 1.73 | -11.08 | 160.90 | 52.03 | 251.52 | 0.8179 | -351.0 | -307.8 | |
| 7.72 | 26.59 | 6.57 | 22.53 | -11.42 | 160.49 | 51.62 | 250.98 | 0.8150 | -736.1 | -540.9 | |
| 0.00 | 1.14 | 0.00 | 0.97 | -12.02 | 160.25 | 51.38 | 250.19 | 0.8145 | 168.0 | 34.3 | |
| 3.77 | -17.00 | 3.19 | -17.00 | -11.66 | 160.11 | 51.24 | 250.56 | 0.8121 | -790.7 | 999999 | |
| 0.00 | 1.93 | 0.00 | 1.57 | -12.44 | 158.28 | 49.41 | 248.96 | 0.7968 | -501.0 | -458.5 | |
| 0.00 | 1.58 | 0.00 | 1.28 | -12.23 | 158.09 | 49.22 | 249.13 | 0.7942 | -581.0 | -534.8 | |
| 0.00 | 1.76 | 0.00 | 1.44 | -13.26 | 158.36 | 49.49 | 248.01 | 0.8003 | -530.0 | -462.7 | |
| 0.00 | 0.97 | 0.00 | 0.78 | -12.48 | 158.06 | 49.19 | 248.82 | 0.7947 | -615.0 | -517.1 | |
| 0.00 | 1.14 | 0.00 | 0.92 | -12.62 | 157.86 | 48.99 | 248.58 | 0.7932 | -753.0 | -617.4 | |
| 0.70 | 1.76 | 0.58 | 1.44 | -14.07 | 158.11 | 49.24 | 246.96 | 0.8007 | -573.1 | -484.9 | |
| 0.00 | 0.79 | 0.00 | 0.63 | -12.31 | 157.54 | 48.67 | 248.83 | 0.7891 | -702.0 | -578.0 | |
| 0.00 | 0.53 | 0.00 | 0.38 | -13.81 | 150.98 | 42.12 | 243.98 | 0.7270 | -190.0 | -186.0 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |